| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1771133 | Astroparticle Physics | 2011 | 7 Pages |
Abstract
⺠Galactic magnetic turbulence are traced by the angular power spectrum of radio maps. ⺠The turbulence power spectrum is found to be flatter than 3D Kolmogorov. ⺠The turbulent halo scale is found to be thin, smaller than (of order of) 1 kpc. ⺠Results point towards non-conventional cosmic-ray models with convective winds. ⺠Alternatively, results can suggest non-trivial mechanism for transferring turbulent energy from large to small scales.
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Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Marco Regis,